Chapter 7: Radiation and Matter Flashcards
Interaction btwn Radiation and Matter
(Hamiltonian)
- Decompose into interacting and non-interacting parts
- NOTE: Assumes Coulomb gauge [A,p]=0
Interaction btwn Radiation and Matter
(Hilbert Space)
Only Hint acts on both spaces
Time-Dependent Perturbation Theory
(Hamiltonian)
- H0 is time-independent and complete eigenbasis is known
- H’(t) is small
Interaction Picture
(Overview)
- Intermediary picture between Schrödinger and Heisenberg
- Expectation values are invariant
Dirac Time-Evolution Operators
Expand UD(t) to get approximations
Interaction Picture
(Wavefunction)
Interaction Picture
(Operators)
Interaction Picture
(Schrödinger Equation)
Interaction Picture
(Summary)
- States evolve under interaction Hamiltonian
- Operators evolve under non-interacting Hamiltonian
Fermi’s Golden Rule
(Transition Probability)
Gives probability for the transition between two states due to external excitation
Fermi’s Golden Rule
(Rate Equation)
Fermi’s Golden Rule
(Rate Equation [Multiple Final States])
ρ(Ei) ≡ density of state at Ei
Hydrogen Atom in Radiation Field
(Assumptions)
- Hailtonian: H = H0 + H’= (Hpart + Hem) + Hint
- Initial state:
- | i > ≡ | a > | n<em>kλ</em> >
- Ei = Ea + (hbar) ωkλnkλ
-
Final state:
- | f > ≡ | b > | n<em>kλ</em> + 1 >
- Ef = Eb + (hbar) ωkλ(nkλ+1) = Ei
Hydrogen Atom in Radiation Field
(Take-Away)
- δ(Ei − Ef) gives that emitted photon must have energy equal to energy difference of final and initial energies
- Transition rate yield expressions for stimulated/sponstaneous emission and stimulated absorptions
- nkλ = 0 → spontaneous emission
- nkλ > 0 → stimulated emission/absorption
Hydrogen Atom in Radiation Field
(Notes)
- ω3/c2 ∈ field
- rab ∈ atom
- fine structure constant α ≡ coupling strength between matter and radiation